arXiv:astro-ph/0702499v1 19 Feb 2007
arXiv:1010.4927v2 [astro-ph.SR] 19 Feb 2011
An l−ν diagram, showing the power spectrum of p-modes sampled 20 km... | Download Scientific Diagram
Local helioseismology and the active Sun
ÈRay paths for modes with a horizontal phase speed of 65 km s~1 in the... | Download Scientific Diagram
Time–Distance Helioseismology Data-Analysis Pipeline for Helioseismic and Magnetic Imager Onboard Solar Dynamics Observatory (
Time-Distance Helioseismology of Sunspots
arXiv:1209.4877v1 [astro-ph.SR] 21 Sep 2012
arXiv:1607.05681v1 [astro-ph.SR] 19 Jul 2016
SYSTEMATIC CENTER-TO-LIMB VARIATION IN MEASURED HELIOSEISMIC TRAVEL TIMES AND ITS EFFECT ON INFERENCES OF SOLAR INTERIOR MERIDIO
arXiv:0911.4295v1 [astro-ph.SR] 22 Nov 2009
Comparison of Travel-Time Definitions
Chapter 3 Near-surface oscillations 3.1 IntroductionW For almost two decades, methods of local helioseismology (e.g, Hill, 1988;
Time Distance Study of Isolated Sunspots – arXiv Vanity
Results of Gabor-wavelet fitting for the central frequency (ω 0 ) for... | Download Scientific Diagram
Implementation and Comparison of Acoustic Travel-Time Measurement Procedures for the Solar Dynamics Observatory/Helioseismic and Magnetic Imager Time – Distance Helioseismology Pipeline | SpringerLink
Inversions for Deep Solar Meridional Flow Using Spherical Born Kernels – arXiv Vanity
Implementation and Comparison of Acoustic Travel-Time Measurement Procedures for the Solar Dynamics Observatory/Helioseismic and
Time Distance Study of Isolated Sunspots – arXiv Vanity
Comparison of acoustic travel-time measurements of solar meridional circulation from SDO/HMI and SOHO/MDI
Response to Comment on “Detection of Emerging Sunspot Regions in the Solar Interior” | Science
Evolution of subsurface flows in active regions
1. INTRODUCTION
Subsurface Supergranular Vertical Flows as Measured Using Large Distance Separations in Time–Distance Helioseismology
Time Distance Study of Isolated Sunspots
